Open Access
Fig. 2
Download original image
Residuals of spin pole solutions from light curve inversion for asteroid (762) Pulcova. The light regions correspond to lower χ2 values, and therefore better-fit solutions. The coordinates of the best-fit orbital pole are marked with a star.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.